Cosmology with the eROSITA all-sky survey of galaxy clusters

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eRosita PSF• 15” on-‐axis HEW (@ 1.5 keV) è 28” <strong>survey</strong>-averagedN. Clerc – Oxford – 17 Sept. 2013PANTER FM2 focal plane measurements @ 1.49 keV (image NC, Panter-‐MPE)

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eRosita effective area and graspEffective Area!Grasp Merloni et al. 2012 “eRosita science book” N. Clerc – Oxford – 17 Sept. 2013

eRosita PSF• 15” on-‐axis HEW (@ 1.5 keV) è 28” <strong>survey</strong>-averagedN. Clerc – Oxford – 17 Sept. 2013PANTER FM2 focal plane measurements @ 1.49 keV (image NC, Panter-‐MPE)

Page 1 and 2: The eRosita X-ray all-sky survey,ga
Page 3 and 4: eRosita collaborationPI: Peter Pred
Page 5: eRosita on SRGART-XCIKIeROSITAMPENa
Page 11 and 12: eRosita all-sky survey (eRASS=8*6 m
Page 13 and 14: eRosita all-sky survey performancee
Page 15 and 16: The X-ray (extragalactic) universeD
Page 17 and 18: Galaxy clusters in the eRASS~100,00
Page 19 and 20: Main cosmological probesCluster 3D
Page 21 and 22: Optical/NIR surveysIKI(R) D/R spli
Page 23 and 24: SKA (and pathfdrs) & galaxy cluster
Page 25 and 26: Euclid & eRosita galaxy clusters (2

Cosmology with the eROSITA all-sky survey of galaxy clusters

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